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J. Hartke

43 papers hereh-index 8209 citations46 works total

Matching runs newest-first, so older work may not be attached to this profile yet.

author position
  • sole author1
  • first author8
  • middle author29
  • last author2

Across the 40 of 43 papers where every author was matched, so the position is known.

fields
  • astro-ph.GA42
  • astro-ph.IM1
same name
  • J. Hartke — 5 papers, h 1
  • J. Hartke — 2 papers, h 2
  • J. Hartke — 2 papers, h 1
  • J. Hartke — 1 paper, h 3
  • J. Hartke — 1 paper, h 2
  • J. Hartke — 1 paper, h 5

Either other researchers who publish under this name, or the same person where the external sources have not merged their records.

identity via Semantic Scholar / OpenAlex

activity
20172026
most citedThe halo of M49 and its environment as traced by planetary nebulae

30 citations · 297 across the 39 of their papers we have counts for

collaborators
Showing 2024Show all

3 papers · 1 filter

astro-ph.GA2024

INSPIRE: INvestigating Stellar Population In RElics -- VII. The local environment of ultra-compact massive galaxies

Diana Scognamiglio, Chiara Spiniello, Mario Radovich +15

Relic galaxies, the oldest ultra-compact massive galaxies (UCMGs), contain almost exclusively "pristine" stars formed during an intense star formation (SF) burst at high redshift.…

astro-ph.GA2024★ 4 cited

Shapes of dark matter haloes with discrete globular cluster dynamics: The example of NGC 5128 (Centaurus A)

Tadeja Veršič, Marina Rejkuba, Magda Arnaboldi +7

Within the ΛCDM cosmology, dark matter haloes are expected to deviate from spherical symmetry. Constraining the halo shapes at large galactocentric distances is challenging due t…

astro-ph.GA2024★ 2 cited

INSPIRE: INvestigating Stellar Population In RElics VI -- The low-mass end slope of the stellar Initial Mass Function and chemical composition

Michalina Maksymowicz-Maciata, Chiara Spiniello, Ignacio Martín-Navarro +9

The INSPIRE project has built the largest sample of ultra-compact massive galaxies (UCMGs) at 0.1<z<0.4 and obtained their star formation histories (SFHs). Due to their preserved v…

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Not affiliated with arXiv. Researcher data from Semantic Scholar (ODC-BY) and OpenAlex.